Results » History » Version 15
PASCHOS, Alexandros, 12/15/2015 03:53 AM
1 | 15 | PASCHOS, Alexandros | h1. *6. Results* |
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2 | 1 | PASCHOS, Alexandros | |
3 | 1 | PASCHOS, Alexandros | When the communication between the USRPs was established, the transmitted constellation below was obtained. |
4 | 1 | PASCHOS, Alexandros | |
5 | 3 | PASCHOS, Alexandros | p=. !{width: 30%}https://sourceforge.isae.fr/attachments/download/1513/Tx_Constellation.png(Transmitted Constellation)! |
6 | 11 | PASCHOS, Alexandros | _Figure 6.1 Transmitted Constellation_ |
7 | 1 | PASCHOS, Alexandros | |
8 | 12 | PASCHOS, Alexandros | Using an IQ sampling of $500k$, obtaining a symbol rate of $62500$ symbols/sec, without any noise, the received constellation is shown below. The $BER$ in this case is, evidently, 0. |
9 | 1 | PASCHOS, Alexandros | |
10 | 3 | PASCHOS, Alexandros | p=. !{width: 30%}https://sourceforge.isae.fr/attachments/download/1511/Rx_Constellation_no_noise.png(Received Constellation)! |
11 | 11 | PASCHOS, Alexandros | _Figure 6.2 Received Constellation without AWGN_ |
12 | 1 | PASCHOS, Alexandros | |
13 | 14 | PASCHOS, Alexandros | The constellation on Figure 6.3 was obtained when adding AWGN, for a target $E_b/N_0$ (received $E_b/N_0$) of 5.The constellation will vary as the values of $E_b/N_0$ vary, making it either noisier, or making it resemble a noiseless channel. |
14 | 1 | PASCHOS, Alexandros | |
15 | 3 | PASCHOS, Alexandros | p=. !{width: 30%}https://sourceforge.isae.fr/attachments/download/1512/Rx%20_Constellation_AWGN.png(Noisy Constellation)! |
16 | 11 | PASCHOS, Alexandros | _Figure 6.3 Noisy Constellation_ |
17 | 1 | PASCHOS, Alexandros | |
18 | 14 | PASCHOS, Alexandros | With AWGN, the $BER$ is calculated, then compared to the theoretical one, obtaining a $BER$ vs $E_b/N_0$ graph like the one depicted below in Figure 6.4. It can be seen that the simulated $BER$ follows, as expected, the same behavior as the theoretical $BER$. |
19 | 1 | PASCHOS, Alexandros | |
20 | 8 | PASCHOS, Alexandros | p=. !{width: 60%}https://sourceforge.isae.fr/attachments/download/1514/BERtheory.jpg(Theroretical an Simulated)! |
21 | 11 | PASCHOS, Alexandros | _Figure 6.4 BER vs Eb/No without coding_ |
22 | 5 | PASCHOS, Alexandros | |
23 | 12 | PASCHOS, Alexandros | The $BER$ is also calculated for a the BCH code or a rate of (roughly) 1/2, and compared to the simulated $BER$ without coding. It can be observed from the graph below, that BCH greatly improves the $BER$. In this case, there is a gain of $3dB$ for a $BER=10^-5$ |
24 | 9 | PASCHOS, Alexandros | |
25 | 10 | PASCHOS, Alexandros | p=. !{width: 60%}https://sourceforge.isae.fr/attachments/download/1516/BERbch.jpg(BCH Coding)! |
26 | 11 | PASCHOS, Alexandros | _Figure 6.5 BER vs Eb/No with BCH coding_ |